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Artist’s Concept of Extrasolar Planet’s Hazy Atmosphere

Artist's Concept of Extrasolar Planet's Hazy Atmosphere
A team of astronomers, led by Frederic Pont from the Geneva University Observatory in Switzerland, has detected for the first time strong evidence of hazes in the atmosphere of a planet orbiting a distant star. The new Hubble Space Telescope observations were made as the extrasolar planet, dubbed HD 189733b, passed in front of its parent star in an eclipse. As the light from the star briefly passes through the exoplanet's atmosphere, the gases in the atmosphere stamp their unique spectral fingerprints on the starlight. Where the scientists had expected to see the fingerprints of sodium and potassium, there were none; implying that high-level hazes (with an altitude of nearly 2,000 miles) are responsible for blocking the light from these elements. This is an artist's concept of HD 189733b and its parent star.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    20h 00m 43s.72
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    +22° 42' 38".6
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Vulpecula
  • Distance
    DistanceThe physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
    Roughly 60 light-years (19 parsecs)

About the Data

  • Data Description
    Data DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
    Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
    This image was created from HST data from proposal 10869: A. Lecavelier des Etangs, A. Vidal-Madjar, F. Bouchy , J.-M. Desert, D. Ehrenreich, R. Ferlet, G. Hebrard, and G. Tinetti (CNRS, Paris Institute of Astrophysics), G. Ballester (University of Arizona), and F. Pont and S. Udry (Geneva University Observatory, Switzerland). The science team comprises: F. Pont (Geneva University Observatory, Switzerland) , H. Knutson (Harvard-Smithsonian Center for Astrophysics), R. Gilliland (STScI), C. Moutou (Astrophysics Laboratory of Marseille, France), and D. Charbonneau (Harvard-Smithsonian Center for Astrophysics).
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>ACS/SBC
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    June, 2007, Exposure Time: 9.5 hours
  • Filters
    FiltersThe camera filters that were used in the science observations.
    110/115 (UV)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    HD 189733, HD189733b
  • Object Description
    Object DescriptionThe type of astronomical object.
    Planet transiting a bright, nearby K0 star
  • Release Date
    December 11, 2007
  • Science Release
    Hubble Finds that Extrasolar Planet Has a Hazy Sunset
  • Credit
    Science: F. Pont (Geneva University Observatory, Switzerland); Image: NASA, ESA, and G. Bacon (STScI)

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Details

Last Updated
Mar 28, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov